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A Study Of (oi) 63.2 And 145.5 Micron Emission From M17 And Sgr A From The Lear Jet by Gary J. Melnick
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1NASA Technical Reports Server (NTRS) 19860021153: A Study Of (OI) 63.2 And 145.5 Micron Emission From M17 And SGR A From The Lear Jet
By NASA Technical Reports Server (NTRS)
The Lear Jet Observatory was used to observe the 157.7 micron (C II) line from the galactic H II regions W3 and W51. These measurements established a lower limit in the 157.7 micron line for solar luminosity of 360 from W3, assuming adistance of 2 kpc, and a solar luminosity of 4100 from W51, assuming a distance of 7 kpc. The data indicated that the CII/far infrared continuum ratio for both W3 and W51 were within the range found for other galactic H II regions.
“NASA Technical Reports Server (NTRS) 19860021153: A Study Of (OI) 63.2 And 145.5 Micron Emission From M17 And SGR A From The Lear Jet” Metadata:
- Title: ➤ NASA Technical Reports Server (NTRS) 19860021153: A Study Of (OI) 63.2 And 145.5 Micron Emission From M17 And SGR A From The Lear Jet
- Author: ➤ NASA Technical Reports Server (NTRS)
- Language: English
“NASA Technical Reports Server (NTRS) 19860021153: A Study Of (OI) 63.2 And 145.5 Micron Emission From M17 And SGR A From The Lear Jet” Subjects and Themes:
- Subjects: ➤ NASA Technical Reports Server (NTRS) - ASTROPHYSICS - HYDROGEN - INTERSTELLAR MATTER - MOLECULAR CLOUDS - RECOMBINATION REACTIONS - STELLAR LUMINOSITY - CARBON - EMISSION SPECTRA - H II REGIONS - LEAR JET AIRCRAFT - LINE SPECTRA - NEBULAE - RESEARCH AIRCRAFT - TELESCOPES - Melnick, G. G.
Edition Identifiers:
- Internet Archive ID: NASA_NTRS_Archive_19860021153
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